This sequence compares Chandra's X-ray image of 3C58 with the views seen by optical and radio telescopes. The intricate X-ray loops in the Chandra image and the features in the radio images of 3C58 extend a dozen light years from the pulsar, likely representing the complex magnetic field structure there.
[Runtime: 0:32](X-ray: NASA/CXC/SAO/P.Slane et al.; Optical: DSS; Radio: NCSU/S.Reynolds)

Chandra's image of the Vela Pulsar shows a dramatic bow-like structure at the leading edge of the cloud, or nebula, embedded in the Vela supernova remnant. As indicated by the arrow, the jets point in the same direction as the motion of the pulsar. The swept-back appearance of the nebula is due to the motion of the pulsar through the supernova remnant. The last few frames of this animation show the region of space around the rapidly rotating neutron stars in the Crab Nebula (left) compared with Vela (right). The inner Crab ring is 1 light year in diameter; in Vela it is 0.1 light year.
[Runtime: 0:16](Animation: NASA/CXC/A.Hobart; Images: NASA/SAO/CXC)

his sequence starts with Chandra's wide-field of the region around the Vela Pulsar Jet. The view then zooms into the area covered by Chandra during a series of 13 observations taken over about two and a half years. This movie led astronomers to discover an outer jet shooting out ahead of the moving pulsar. The most striking feature of the jet is its variability, changing both its shape and brightness. Meanwhile, bright blobs are seen moving along the jet with surprising velocities -- at about half of the speed of light.
[Runtime: 1:16](Animation: NASA/CXC/Penn State/G.Pavlov et al.)

Beginning with a wide-field view of the supernova remnant IC 443, this sequence moves into a closer look at the neutron star embedded within known as J0617. The images show these objects in X-rays (blue), radio (green), and optical (red). The location and orientation of J0617's wake are mysterious for astronomers who would have expected it to be aligned toward the center of IC 443.
[Runtime: 0:32](Chandra X-ray: NASA/CXC/B.Gaensler et al; ROSAT X-ray: NASA/ROSAT/Asaoka & Aschenbach; Radio Wide: NRC/DRAO/D.Leahy; Radio Detail: NRAO/VLA; Optical: DSS)

This sequence begins with an artist's animation of the explosion that produced the Crab Nebula, now an expanding debris field of extremely high-energy particles created from the death of a massive star. The view then fades into an image of the Crab composed of data from Chandra (light blue), Hubble (green and dark blue), and Spitzer (red).
[Runtime: 0:18](Animation: ESA/Hubble/M. Kornmesser & L. L. Christensen Image: X-ray: NASA/CXC/ASU/J.Hester et al.; Optical: NASA/ESA/ASU/J.Hester & A.Loll; Infrared: NASA/JPL-Caltech/Univ. Minn./R.Gehrz)